ALMA-IMF - XI. The sample of hot core candidates: A rich population of young high-mass protostars unveiled by the emission of methyl formate

Open Access

Fig. 11

Methyl formate source size distribution derived fitting 2D Gaussians to the CH₃OCHO moment 0 maps using GExt2D. The non-deconvolved (FWHM_mf) and deconvolved sizes ( ${F W H M}_{M F}^{d e c}$ $\[\mathrm{FWHM}_{\mathrm{MF}}^{\mathrm{dec}}\]$ ) are shown in blue and red, respectively. The green dotted line shows the median of the deconvolved source sizes, while the dashed purple line shows the median beam size of the line cubes.

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